The LISA interferometer is planned to launch in 2034, with the noise power spectral density well approximated
by [1]}, [2]}
\(S_{\rm LISA}(f)=\frac{10}{3L^2}\left( P_{\rm OMS}(f)+2\left[ 1+\cos ^2\left( \frac{f}{f_{\ast }} \right) \right]\frac{P_{\rm acc}(f)}{(2\pi f)^4} \right)\left[ 1+\frac{6}{10}\left( \frac{f}{f_{\ast }} \right)^2 \right]+S_c(f),~~~~\) 
